Hello Markus,
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Originally Posted by Stonius
Hi Steven, sorry for the late reply - I've been away. Also, I've been trying to get what you're saying - I'm not particularly mathematical. So let me see if I have this right?
So you're saying my idea would not be linear as is observed in nature, but would instead be, what, logarithmic?
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The mathematics is to show the non linearity of recession velocity vs distance for an object travelling through space if acceleration is present without having to know the specific values for acceleration.
This will become clearer below.
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Which is interesting because if spacetime expands only in the absence of matter, then you would assume that the gravitational force has limited range, or falls off in a way we don't understand, which would have implications for dark matter, one would have thought.
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In the early Universe there was no matter in the form of atoms, molecules, stars, and galaxies but gravity still existed.
Where as gravity requires the presence of mass in the Newtonian model, mass and energy are the requirements for gravity in General Relativity.
In the early Universe most of the energy was carried by photons and neutrinos travelling at relativistic velocities in a radiation dominated Universe which was followed by a matter dominated Universe (including dark matter) which gave way to a dark energy dominated Universe from about six billion years ago.
The difference of each stage of the Universe relates to the how expansion varies as a function of time.
https://en.wikipedia.org/wiki/Scale_factor_(cosmology)
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Why non-relativistic? Isn't the whole point of the Observable universe's event horizon that it recedes from us at relativistic velocities? That's why we can never see past it?
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As strange as it appears objects that have a recession velocity due to space expansion that exceed c, the speed of light, are no longer “relativistic” because the equations for special relativity don’t apply.
In this case if an object is travelling at a recession velocity v which exceeds c and a photon is emitted by the object back towards the observer at a speed c, the observer will only see the object if the vector equation is v-c<c.
In the case of your example for objects moving in space it is mathematically simpler to deal with Newtonian time and slower speeds without having to worry about time dilation.
Mathematically this is a good approximation for velocities up to about 90% the speed of light.
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So why can't we just use a = Δv / Δt if we're talking non-relativistic velocities, or a 4-vector for relativistic velocities? I'm not sure why the higher order derivatives are necessary, or why you begin by multiplying Velocity and time instead of dividing delta time by delta velocity. Sorry for my ignorance. Which acceleration equation are you using?
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The equation
a = Δv / Δt is only valid if the acceleration is constant.
If the acceleration is not constant as your idea suggests then Δv / Δt will vary at any given location.
The equation
x=vt+(dv/dt)t^2/2!+(d^2v/dt^2)t^3/3!+(d^3v/dt^3)t^4/4+...... is known as the Taylor expansion of a function.
Many functions can be broken down into this series and expressed to any given degree of accuracy depending on the number of terms in the expansion.
Consider the equation
dv/dt=d2x/dt2=0 which is the equation for zero acceleration.
Integrating this equation gives
dx/dt=v where v is the velocity.
Integrating further gives
x=vt, where x is the position at time t for an object moving at constant velocity v.
Note this is the first term in the Taylor expansion.
Since there is no v^2 or higher term (or any term other than the power of one) there is a linear relationship between x and v at any time t.
Despite the linear relationship, it bears no resemblance to the recession velocity distance relationship in Hubble’s law as it has a zero gradient due to the constant velocity.
Incorporating acceleration into the picture doesn’t help either.
Consider the equation
dv/dt=d2x/dt2=a where a is uniform or constant acceleration.
Integrating gives
dx/dt=at+v
Integrating again gives
x=(a)t^2/2+vt
=vt+(a)t^2/2
=vt+(dv/dt)t^2/2!
Note we now have the first two terms in the Taylor expansion.
If the acceleration is not constant the Taylor expansion incorporates more terms, the higher the accuracy the more terms are required.
Eliminating t from the equation dv/dt=a for constant acceleration shows the non linearity between v and x.
dv/dt=(dx/dt)(dv/dx) by the chain rule
=vdv/dx
=d/dv(1/2v^2)dv/dx
=d(1/2v^2)/dx
Hence
d(1/2v^2)/dx=a
Integrating gives
1/2v^2=ax+u^2/2 where u is the initial velocity.
Hence
v^2= 2ax+u^2
Clearly there is no linear relationship between v and x because of the v^2 term.
Any constant acceleration will destroy the linear relationship between v and x.
A variable acceleration which includies higher terms in the Taylor expansion will also result in non linearity.
Hence we don’t need to specifically know the acceleration to indicate the non linear relationship between v and x.
For objects moving in space, it is impossible to reproduce Hubble’s law
Hope this clears it up.
Steven